Difference between revisions of "Lunar outgassing"

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Outgassing events in which [[radon]], [[nitrogen]], and [[carbon dioxide]] are vented to the surface, may be the result of low level volcanic or tectonic events on the moon, and are hypothesized to be the source of the extremely thin lunar atmosphere.
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Outgassing events in which [[radon]], [[nitrogen]], [[carbon monoxide]], and [[carbon dioxide]] from deepo in the lunar interior are vented to the surface may be the result of low level volcanic or tectonic events on the moon, and are hypothesized to be the source of the extremely thin lunar atmosphere.  Understanding when and where these events occur may help us understand more about lunar tectonics and how the moon's atmosphere was formed.
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[[Carbon]] and [[Nitrogen]] are both vital elements which will have to be imported from earth.  If outgassing events can be predicted it may be possible to [[ISRU|utilize]] this valuable resource.
  
 
The [[Alpha Particle Spectrometer]] aboard [[Lunar Prospector]] was designed to detect these events by tracking the [[alpha particle|alpha particles]] emitted during the decay of radon and [[polonium]] (a daughter element in it's decay series).  The APS data was obscured by solar activity during the mission, but may be viewable once the effects of solar activity have been filtered out.  This task has not been done.
 
The [[Alpha Particle Spectrometer]] aboard [[Lunar Prospector]] was designed to detect these events by tracking the [[alpha particle|alpha particles]] emitted during the decay of radon and [[polonium]] (a daughter element in it's decay series).  The APS data was obscured by solar activity during the mission, but may be viewable once the effects of solar activity have been filtered out.  This task has not been done.
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[[Category:Selenology]]

Revision as of 11:15, 20 February 2007

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Outgassing events in which radon, nitrogen, carbon monoxide, and carbon dioxide from deepo in the lunar interior are vented to the surface may be the result of low level volcanic or tectonic events on the moon, and are hypothesized to be the source of the extremely thin lunar atmosphere. Understanding when and where these events occur may help us understand more about lunar tectonics and how the moon's atmosphere was formed.

Carbon and Nitrogen are both vital elements which will have to be imported from earth. If outgassing events can be predicted it may be possible to utilize this valuable resource.

The Alpha Particle Spectrometer aboard Lunar Prospector was designed to detect these events by tracking the alpha particles emitted during the decay of radon and polonium (a daughter element in it's decay series). The APS data was obscured by solar activity during the mission, but may be viewable once the effects of solar activity have been filtered out. This task has not been done.